Recent activity

The geomagnetic field was quiet on April 20. Solar wind
speed ranged between 306 and 371 km/sec. A weak (likely coronal hole based) disturbance arrived at SOHO near 22:30 UTC and this
caused a fairly slow increase in wind speed to near 450 km/sec early on April 21. The interplanetary magnetic field was mostly
northwards until 02h UTC, the swung southwards until 04h UTC.

Solar flux measured at 20h UTC on 2.8 GHz was 110.7. The planetary A
index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 5.8).
Three hour interval K indices: 11122212 (planetary), 21223212 (Boulder).

The background x-ray flux is at the class B1 level.

At midnight there were 5 spotted regions on the visible disk. The solar flare activity level was very low. No C class events
were recorded during the day.

Region 10593 decayed further and could become spotless within 2 days if the current rate of decay is sustained.
Region 10596 decayed in the leading spot section where a magnetic delta structure disappeared. Slow development was
observed in the trailing spot section and a magnetic delta formed in the northwestern part. A minor M class flare is
possible.
New region 10597 emerged in the southwest quadrant.

Spotted regions not numbered by NOAA/SEC:[S391] This region emerged to the north of region 10595 late on April 16 and developed moderately quickly on April 17.
Further development was observed on April 18, while the region decayed slowly on April 19 and lost several small spots. The region
decayed further on April 20. Location at
midnight: S06E13.
[S394] A new region emerged late on April 19 in the southwest quadrant near the center of the visible disk and added a few
spots on April 20. Location at midnight: S07W16.

Coronal mass ejections (CMEs)

April 18-20: No fully or partly Earth directed CME observed. A full halo CME observed on April 20 had a backsided origin.

Coronal holes

The northernmost extensions of a coronal hole (CH91) in the southern hemisphere were in a geoeffective position on
April 19-20. A recurrent coronal hole (CH92) in the northern hemisphere will probably rotate into a geoeffective position on April
22-24.

Processed SOHO/EIT 284 image at 19:05 UTC on April 20. The darkest areas on the solar disk are likely coronal holes.

Forecast

The geomagnetic field is expected to be quiet to unsettled on April 21 and quiet to active on April 22-23 due to a weak high speed stream
from coronal hole CH91.

Long distance low and medium frequency (below 2 MHz) propagation along
east-west paths over high and upper middle latitudes was good before 03:30 UTC, then became fair due to the influence from the
current weak disturbance. Propagation along long distance north-south paths is fair to poor. [Trans
Atlantic propagation conditions are currently monitored every night on 1470 kHz. Dominant stations tonight: Radio Vibración
(Venezuela) and WLAM Lewiston ME. On other frequencies lots of stations from the eastern parts of Canada and USA were heard,
especially prior to 03:30 UTC].

Coronal holes (1)

Coronal mass ejections (2)

M and X class flares (3)

1) Effects from a coronal hole could reach Earth within the next 5 days. When the high speed stream has arrived
the color changes to green.
2) Material from a CME is likely to impact Earth within 96 hours.
3) There is a possibility of either M or X class flares within the next 48 hours.

Data for all numbered solar regions according to the Solar Region Summary provided by
NOAA/SEC. Comments are my own, as is the
STAR spot count (spots observed at or inside a few hours before midnight) and data for regions not numbered by SEC or where SEC has observed no spots.
SEC active region numbers in the table below and in the active region map above are the historic
SEC/USAF numbers.

Active region

Date numbered

SEC
spot
count

STAR
spot
count

Location at midnight

Area

Classification

Comment

10592

2004.04.13

S10W34

plage

10593

2004.04.14

9

5

S19W37

0060

DSO

area was 0030
at midnight

10594

2004.04.14

1

N15W13

0020

HSX

spotless

10595

2004.04.16

10

S07E13

0070

DAO

spotless
instead of numbering a
new region, SEC has
reused 10595. See
S391

10596

2004.04.18

20

19

S09E31

0340

DKO

beta-gamma-delta

10597

2004.04.20

6

3

S06W60

0070

DAO

classification was DSO
at midnight, area 0050

S388

emerged on
2004.04.12

S07W49

plage

S391

emerged on
2004.04.16

7

S06E13

0060

DAO

S393

emerged on
2004.04.18

N07W20

plage

S394

emerged on
2004.04.19

4

S07W16

0010

BXO

Total spot count:

46

38

SSN:

96

88

Monthly solar cycle data

Month

Average solar
flux at Earth

International sunspot number

Smoothed sunspot number

2000.04

184.2

125.5

120.8
cycle 23 sunspot max.

2000.07

202.3

170.1

119.8

2001.12

235.1

132.2

114.6 (-0.9)

2003.03

131.4

61.1

74.0 (-4.3)

2003.04

126.4

60.0

70.1 (-3.9)

2003.05

115.7

55.2

67.6 (-2.5)

2003.06

129.3

77.4

65.0 (-2.6)

2003.07

127.7

83.3

61.8 (-3.2)

2003.08

122.1

72.7

60.0 (-1.8)

2003.09

112.2

48.7

59.5 (-0.5)

2003.10

151.7

65.5

(58.0 predicted, -1.5)

2003.11

140.8

67.3

(55.9 predicted, -2.1)

2003.12

114.9

46.5

(53.3 predicted, -2.6)

2004.01

114.1

37.2

(49.1 predicted, -4.2)

2004.02

107.0

46.0

(44.5 predicted, -4.6)

2004.03

112.0

48.9

(41.7 predicted, -2.8)

2004.04

100.5 (1)

41.3 (2)

(39.6 predicted, -2.1)

1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz.
2) Unofficial, accumulated value based on the Boulder (NOAA/SEC) sunspot number. The official international sunspot number is typically
30-50% less.

This report has been prepared by Jan
Alvestad. It is based partly on my own observations and analysis, and
partly on data from some of these solar data sources. All time references are to the UTC day. Comments and suggestions are always welcome.